SIMBAD references

A. Arai, Kyoto Sangyo University, reports that an optical spectrogram (resolution 500) of the variable was obtained using the 1.3-m ARAKI telescope on May 8.66 UT under poor sky conditions. The spectrum shows a blue continuum and a weak H-alpha emission line (EW about 0.4 nm), suggesting that the object would be classified as a dwarf nova. No other significant emission or absorption lines were seen in the low-S/N data.